Quintessential inflation with a trap and axionic dark matter

Dimopoulos, Konstantinos and Owen, Charlotte and Karciauskas, Mindaugas (2019) Quintessential inflation with a trap and axionic dark matter. Physical Review D, 100 (8). ISSN 1550-7998

[img] Text (1907.04676)
1907.04676.pdf - Published Version
Available under License Creative Commons Attribution.

Download (806kB)


We study a new model of quintessential inflation which is inspired by supergravity and string theory. The model features a kinetic pole, which gives rise to the inflationary plateau, and a runaway quintessential tail. We envisage a coupling between the inflaton and the Peccei-Quinn (PQ) field which terminates the roll of the runaway inflaton and traps the latter at an enhanced symmetry point (ESP), thereby breaking the PQ symmetry. The kinetic density of the inflaton is transferred to the newly created thermal bath of the hot big bang due to the decay of PQ particles. The model successfully accounts for the observations of inflation and dark energy with natural values of the model parameters, while also resolving the strong CP problem of QCD and generating axionic dark matter, without isocurvature perturbations. Trapping the inflaton at the ESP ensures that the model does not suffer from the infamous 5th force problem, which typically plagues quintessence.

Item Type: Journal Article
Journal or Publication Title: Physical Review D
Uncontrolled Keywords: /dk/atira/pure/subjectarea/asjc/3100
Departments: Faculty of Science and Technology > Physics
ID Code: 138166
Deposited By: ep_importer_pure
Deposited On: 23 Oct 2019 13:55
Refereed?: Yes
Published?: Published
Last Modified: 16 Feb 2020 05:24
URI: https://eprints.lancs.ac.uk/id/eprint/138166

Actions (login required)

View Item View Item